In particular, one question concerns the survival of the structure
of Kasner epochs connected by quick transitions,
and whether they follow the same transition rules as in the classical picture.
In this paper, we analyze this question within the context of a simple locally rotationally symmetric (LRS) Bianchi II model.
We first analyze the canonical structure and exact solutions of the classical model,
identifying the transition rules of the canonical variables of the system.
Then we develop an exact quantization of the model and
focus on analyzing the survival of
the Kasner transition and the quantum modification of the transition rules.
For such a purpose, we will perform a decomposition of the wavefunction into its
infinite set of moments following the framework first presented in [1]}.
This formalism is very useful to understand the dynamics of peaked semiclassical states
and it has already been applied to the analysis of a variety of cosmological models; see, e.g., [2]}–[3]}.
